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Cline 210 $aWashington$cThe MIT Press$d1984 215 $a317 p.$d24 cm. 606 $aSviluppo economico$2FI 606 $aDebiti$2FI 676 $a336.3409$v21 700 1$aCLINE,$bWilliams R.$0613675 801 $aIT$bSOL$c20120104 912 $a990005458820203316 950 $aDIP.TO SCIENZE ECONOMICHE - (SA)$dDS 300 336.3409 CLI$e1406 DISES 951 $a300 336.3409 CLI$b1406 DISES 959 $aBK 969 $aDISES 979 $c20121027$lUSA01$h1532 979 $c20121027$lUSA01$h1613 996 $aSystemic risk and policy response$91127856 997 $aUNISA NUM $aUSA5928 LEADER 05363nam 2200637 a 450 001 9910438124703321 005 20200520144314.0 010 $a1-283-62403-6 010 $a9786613936486 010 $a1-4614-4400-4 024 7 $a10.1007/978-1-4614-4400-8 035 $a(CKB)2670000000246608 035 $a(EBL)1030553 035 $a(OCoLC)810933669 035 $a(SSID)ssj0000767068 035 $a(PQKBManifestationID)11423976 035 $a(PQKBTitleCode)TC0000767068 035 $a(PQKBWorkID)10733096 035 $a(PQKB)11688897 035 $a(DE-He213)978-1-4614-4400-8 035 $a(MiAaPQ)EBC1030553 035 $a(PPN)168300095 035 $a(EXLCZ)992670000000246608 100 $a20120806d2013 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 13$aAn introduction to waves and oscillations in the sun /$fA. Satya Narayanan 205 $a1st ed. 2013. 210 $aNew York $cSpringer$d2013 215 $a1 online resource (231 p.) 225 0$aAstronomy and astrophysics library,$x0941-7834 300 $aDescription based upon print version of record. 311 $a1-4899-9596-X 311 $a1-4614-4399-7 320 $aIncludes bibliographical references and index. 327 $aChapter 1: Introduction -- 1.1: Historical Perspectives -- 1.2: The Core of the Sun -- 1.3: Radiative Zone -- 1.4: Convection Zone -- 1.5: Photosphere -- 1.6: Chromosphere -- 1.7: Corona -- 1.8: Solar Wind -- Chapter 2: Electro-Magneto Statics -- 2.1: Charge and Current Distributions -- 2.2: Coulomb's Law -- 2.3: Gauss's Law -- 2.4: Ampere's Law -- 2.5: Faraday's Law -- 2.6: Vector Magnetic Potential -- 2.7: Maxwell's Equations -- Chapter 3: MHD Equations and Concepts -- 3.1: Assumptions -- 3.2: Dimensionless Parameters -- 3.3: Mass Continuity -- 3.4: Equations of Motion -- 3.5: Energy Equation -- 3.6: MHD Equilibrium -- 3.7: Magnetic Flux Tubes -- 3.8: Current-free (Potential) fields -- 3.9: Force-Free Fields -- 3.10: Parker's Solution for Solar Wind -- Chapter 4: Waves in Uniform Media -- 4.1: Basic Equations -- 4.2: SoundWaves -- 4.3: Alfv'enWaves -- 4.4: Shear Alfv'enWaves -- 4.5: Compressional Alfv'enWaves -- 4.6: Magneto acoustic Waves -- 4.7: Internal and Magneto acoustic Gravity Waves -- 4.8: Phase-Mixing and Resonant Absorption of Waves -- Chapter 5: Waves in Non-Uniform Media- 5.1: Waves at Magnetic Interface -- 5.2: Surface and InterfacialWaves -- 5.3: Waves in a Magnetic Slab -- 5.4: Waves in Cylindrical Geometries -- 5.5: Waves in Untwisted and Twisted Tubes -- Chapter 6: Instabilities -- 6.1: Introduction -- 6.2: Rayleigh-Taylor (RT) Instability -- 6.3: Kelvin-Helmholtz (KH) Instability -- 6.4: Parametric Instability -- 6.5: Parker Instability -- Chapter 7: Waves in the Sun -- 7.1: Five minute oscillations -- 7.2: Oscillations in Sunspots -- 7.3: Chromospheric Oscillations -- 7.4: CoronalWaves -- 7.5: Coronal Seismology -- 7.6: Coronal Heating due to Waves -- 7.7: EIT and MoretonWaves -- Chapter 8: Heliosesimology -- 8.1: Equations of Motion -- 8.2: Equilibrium Structure -- 8.3: Perturbation Analysis -- 8.4: Acoustic Waves -- 8.5: Internal Gravity Waves -- 8.6: Equations of Linear Stellar Oscillations -- 8.7: Properties of Solar Oscillations (Internal) -- 8.8: p and g modes -- References -- Index. 330 $aAstrophysicists and others studying the Sun will find this expansive coverage of what we know about waves and oscillations in our nearest star an informative introduction to a hot contemporary topic. After a section summarizing the Sun's physical characteristics, the volume moves on to explore the basics of electrodynamics, which in turn facilitate a discussion of magnetohydrodynamics (MHD). The material also details the often complex nature of waves and oscillations in uniform and non-uniform media, before categorizing the observational signatures of oscillations and exploring the instabilities in fluid, dealing with a range of known forms. Lastly, a section on helioseismology explores our growing familiarity with the internal structure of the Sun. This book is a unified portal to a thorough grounding in solar waves that includes a wealth of explanatory vignettes demystifying concepts such as flux tubes, current-free and force-free magnetic fields, the prominences, and the relationship between the vorticity and the induction equation. It also sets out the elegant Parker solution describing the phenomenon of solar wind. The volume will inspire readers with the unbridled enthusiasm of astrophysicists who view the Sun as a giant natural plasma laboratory, in interstellar terms located right on our doorstep, in which they can apply and then verify experimental and theoretical studies on plasma through their own observation. 410 0$aAstronomy and Astrophysics Library,$x0941-7834 606 $aSolar oscillations 606 $aSolar radiation 606 $aSolar radio emission 615 0$aSolar oscillations. 615 0$aSolar radiation. 615 0$aSolar radio emission. 676 $a523.7 700 $aNarayanan$b A. Satya$0916042 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910438124703321 996 $aAn Introduction to Waves and Oscillations in the Sun$92053549 997 $aUNINA